English
Related papers

Related papers: An evolved donor star in the long-period cataclysm…

200 papers

We report near-infrared radial velocity measurements of the recently identified donor star in the high mass X-ray binary system OAO 1657-415 obtained in the H band using ISAAC on the VLT. Cross-correlation methods were employed to construct…

Solar and Stellar Astrophysics · Physics 2015-05-27 A. B. Mason , J. S. Clark , A. J. Norton , P. A. Crowther , T. M. Tauris , N. Langer , I. Negueruela , P. Roche

A large number of white dwarf and donor masses in cataclysmic variables have been found via modelling the primary eclipse, a method that relies on untested assumptions. Recent measurements of the mass of the white dwarf in the cataclysmic…

Solar and Stellar Astrophysics · Physics 2023-11-14 S. P. Littlefair , Pablo Rodríguez-Gil , T. R. Marsh , S. G. Parsons , V. S. Dhillon

We find that the ROSAT source 1RXS J105010.3-140431 is a cataclysmic variable with orbital period of 88.6 minutes and a spectrum closely resembling WZ Sge. In particular, emission lines are flanked by Stark-broadened absorption wings…

Astrophysics · Physics 2009-11-06 R. E. Mennickent , M. Diaz , W. Skidmore , C. Sterken

We present high-speed, three-colour photometry of the eclipsing cataclysmic variable SDSS J170213.26+322954.1 (hereafter SDSS J1702+3229). This system has an orbital period of 2.4 hours, placing it within the ``period gap'' for cataclysmic…

Astrophysics · Physics 2009-11-11 S. P. Littlefair , V. S. Dhillon , T. R. Marsh , B. T. Gaensicke

Cataclysmic variables were long considered to be close binaries consisting of a white dwarf and a Roche-lobe-filling, near-zero-age main-sequence (ZAMS) red or brown dwarf. Recent massive surveys have uncovered an increasing number of…

We present high-speed, three-colour photometry of the eclipsing cataclysmic variable SDSS J150722.30+523039.8 (hereafter SDSS J1507). This system has an orbital period of 66.61 minutes, placing it below the observed ``period minimum'' for…

Astrophysics · Physics 2009-11-13 S. P. Littlefair , V. S. Dhillon , T. R. Marsh , B. T. Gaensicke , I. Baraffe , C. A. Watson

We present the first dynamical determination of the binary parameters of an eclipsing SW Sextantis star in the 3-4 hour orbital period range during a low state. We obtained time-resolved optical spectroscopy and photometry of HS 0220+0603…

We present the analysis of 200 high-resolution and 150 low-resolution spectra of the pulsating subdwarf close binary KPD 1930+2752 obtained with the Keck and the Calar Alto 2.2 m telescopes. Using metal-rich, line blanketed LTE model…

Astrophysics · Physics 2007-05-23 S. Geier , U. Heber , N. Przybilla , R. P. Kudritzki

Intermediate resolution (0.5-1 Angs) optical spectroscopy of the cataclysmic variable SY Cnc reveals the spectrum of the donor star. Our data enable us to resolve the orbital motion of the donor and provide a new orbital solution, binary…

Solar and Stellar Astrophysics · Physics 2015-05-13 J. Casares , I. G. Martinez-Pais , P. Rodriguez-Gil

We present here the results of astrometric, photometric and spectroscopic observations leading to the determination of the orbit and dynamical masses of the binary L dwarf 2MASSW J0746425+2000321. High angular resolution observations spread…

We have obtained simultaneous photometric and spectroscopic observations of the cataclysmic variable 1RXS J064434.5+334451. We have calibrated the spectra for slit losses using the simultaneous photometry allowing to construct reliable…

Solar and Stellar Astrophysics · Physics 2016-10-26 J. V. Hernández Santisteban , J. Echevarría , R. Michel , R. Costero

We present the first reliable determination of the orbital period of the recurrent nova V2487 Oph (Nova Oph 1998). We derived a value of $0.753 \pm 0.016$ d ($18.1 \pm 0.4$ h) from the radial velocity curve of the intense He II…

We present modeling of the long-term optical light curve and radial velocity curve of the binary stellar system CXOGBS J175553.2-281633, first detected in X-rays in the \textit{Chandra} Galactic Bulge Survey. We analyzed 7 years of optical…

We report time-series photometry of the quiescent optical counterpart of the EUV transient RE J1255+266. The star appears as a DA white dwarf with bright emission lines and a complex spectrum of periodic signals in its light curve. A signal…

Astrophysics · Physics 2009-11-10 Joseph Patterson , John Thorstensen , Jonathan Kemp

We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXSJ173021.5-055933, together with simultaneous UV and coordinated optical photometry aiming at…

We have performed detailed numerical calculations of the non-conservative evolution of close binary systems with low-mass (1.0-2.0 M_sun) donor stars and a 1.3 M_sun accreting neutron star. Rather than using analytical expressions for…

Astrophysics · Physics 2007-05-23 T. M. Tauris , G. J. Savonije

We present a new dynamical study of the black hole X-ray transient GRS1915+105 making use of near-infrared spectroscopy obtained with X-shooter at the VLT. We detect a large number of donor star absorption features across a wide range of…

High Energy Astrophysical Phenomena · Physics 2015-06-15 D. Steeghs , J. E. McClintock , S. G. Parsons , M. J. Reid , S. Littlefair , V. S. Dhillon

We present high speed photometric observations of 20 faint cataclysmic variables, selected from the Sloan Digital Sky Survey and Catalina catalogues. Measurements are given of 15 new directly measured orbital periods, including four…

Solar and Stellar Astrophysics · Physics 2015-06-03 Patrick A. Woudt , Brian Warner , Deanne de Bude , Sally Macfarlane , Matthew P. E. Schurch , Ewald Zietsman

We present an analysis of the binary and physical parameters of a unique pulsating white dwarf with a main-sequence companion, SDSS J1136+0409, observed for more than 77 d during the first pointing of the extended Kepler mission: K2…

Splaver and coworkers have measured the masses of the white dwarf and the neutron star components of the PSR J1713+0747 binary system pair by Shapiro Delay. We attempt to find the original configuration of this system performing a set of…

Astrophysics · Physics 2009-06-16 O. G. Benvenuto , R. D. Rohrmann , M. A. De Vito